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  • 1
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    In:  Journal of Seismology, Luxembourg, Conseil de l'Europe, vol. 4, no. 4, pp. 555-565, pp. B04313, (ISBN: 0-12-018847-3)
    Publication Date: 2000
    Keywords: Site amplification ; noksp ; JOSE
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  • 2
    Publication Date: 2000
    Keywords: Strong motions ; Site amplification ; hard ; rock ; Fault zone ; noksp ; JOSE
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  • 3
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    In:  Geophys. Res. Lett., Hannover, Conseil de l'Europe, vol. 25, no. 15, pp. 2877-2880, pp. L04301, (ISSN: 1340-4202)
    Publication Date: 1998
    Description: Propagation of shear waves produced by 25 mantle earthquakes (80-600 km depth) in the subduction zone of the south Tyrrhenian Sea (southern Italy) has been investigated to infer the geometry and extent of the descending lithosphere. From all hypocentral depths high-frequency, high-amplitude shear waves are recorded at most of the stations in southern Italy and easternmost Sicily. This shear-wave energy is interpreted to travel as a guided wave within the descending slab. In contrast, shear waves are either not recorded at all or they are recorded as low-frequency, low-amplitude signals at stations located in the peninsular part of Italy north of the Calabrian arc, in western Sicily and in Sardinia. This systematic S-wave attenuation is interpreted in terms of an active and continuous slab correlated with and limited to the Calabrian arc.
    Keywords: High frequency ... ; Wave propagation ; Hypocentral depth ; Italy ; Subduction zone ; Seismicity ; Shear waves ; GRL
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  • 4
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    In:  Geophys. Res. Lett., Hannover, Conseil de l'Europe, vol. 23, no. 7, pp. 709-712, pp. L04301, (ISSN: 1340-4202)
    Publication Date: 1996
    Description: Pn phases recorded by 40 stations of the Italian seismic network are analyzed using the spectral ratio technique to estimate the Q structure of the uppermost mantle beneath the Italian peninsula and nearby Adriatic Sea. A total of 344 digital waveforms are analyzed from 22 earthquakes that occurred within distances of 300 to 1600 km. The calculated apparent Q values are grouped into two categories: Q〉800 characterizes the Adriatic side of the Italian peninsula, indicating that the Adriatic lithosphere is very efficient in propagating Pn phases through the uppermost mantle; Q〈600 characterizes the uppermost mantle beneath the Apennines and western Italy, indicating less efficient wave propagation. The presence of asthenospheric mantle material at shallow depths beneath the Apennines can explain the observed Q.
    Keywords: Inhomogeneity ; Wave propagation ; P-waves ; earth mantle ; Attenuation ; 7205 ; Seismology: ; Continental ; crust ; (1242) ; Quality factor ; GRL ; 7218 ; Seismology: ; Lithosphere ; and ; upper ; mantle
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  • 5
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    In:  Computers & Geosciences, Oslo, Wiley, vol. 21, no. 2, pp. 279-288, pp. 1604, (ISSN: 1340-4202)
    Publication Date: 1995
    Keywords: Data analysis / ~ processing ; Discrimination ; Detectors ; Seismology
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  • 6
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    In:  J. Geophys. Res., Bonn, Hungarian Academy of Science, vol. 108, no. B3, pp. 10.1-10.14, pp. B04102, (ISBN: 0-12-018847-3)
    Publication Date: 2003
    Keywords: Site amplification ; Strong motions ; Fault zone ; Wave propagation ; Radiation pattern ; noksp ; JGR
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  • 7
    Publication Date: 2011-08-24
    Description: The condensation of solid materials from the vapor phase is important in several scientific fields such as chemical vapor deposition, air pollution and the formation of refractory cosmic dust around stars. Conventional studies of refractory grain formation, using high temperature furnace and shock tube techniques, are restricted to short time scales and suffer from buoyancy induced convection that limit their accuracy. In order to simulate more accurately the condensation of refractory grains near stars and to investigate the advantages of performing condensation studies in microgravity conditions, an experimental investigation was undertaken. This work reports the experimental equipment currently used. The results from the first flight series and particle aggregation modelling efforts are presented briefly.
    Keywords: ASTROPHYSICS
    Type: Microgravity Science and Technology (ISSN 0938-0108); 6; 2; p. 123-130.
    Format: text
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  • 8
    Publication Date: 2013-08-29
    Description: The aim, activity, and some preliminary results of the STARDUST program are presented. The condensation of solid materials from the vapor phase is important in several scientific fields such as chemical vapor deposition, air pollution, and the formation of refractory cosmic dust around stars. Conventional studies of refractory grain formation, using high temperature furnace and shock tube techniques, are restricted to short time scales and suffer from buoyancy induced convection that limit their accuracy. In order to simulate more accurately the condensation of refractory grains near stars and to investigate the advantages of performing condensation studies in microgravity conditions, an experimental investigation of vapor phase condensation in microgravity was undertaken. The experimental equipment currently used is reported. The results from the first flight series and particle aggregation modeling efforts are presented.
    Keywords: MATERIALS PROCESSING
    Type: ESA, Proceedings of the 8th European Symposium on Materials and Fluid Sciences in Microgravity, Volume 2; p 481-488
    Format: text
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  • 9
    Publication Date: 2013-08-29
    Description: A short description of the program Stardust whose goal is to study the formation and properties of high temperature particles and gases, including silicate and carbonaceous materials, that are of interest in astrophysics and planetary science, is given. The international program was carried out in microgravity conditions in parabolic flight. A description of the laboratory equipment, conceived to perform experimental tests in reduced gravity conditions, and which is based on the gas evaporation technique, is given. The gas evaporation technique utilizes one or more heated crucible to vaporize solids materials (SiO, Mg) in a low pressure of inert or reactive gas inside of a vacuum bell jar. The vapor pressures of the materials are controlled by the temperature of the crucibles. The temperature and pressure of inert gas are also controlled. By varying the vapor pressure relative to the gas temperature and pressure, the conditions for substantial grain condensation can be controlled and grain formation measured using light scattering techniques. Thus the partial pressure for grain condensation, can be measured as a function of temperature. The gas evaporation technique has the advantage that complex chemical systems can be studied by using multiple crucibles each containing solid source material. Experimental results and future trends are addressed.
    Keywords: ASTROPHYSICS
    Type: ESA, Environment Observation and Climate Modelling Through International Space Projects. Columbus Eight (COSY-8): Utilisation of Earth Orbiting Laboratories; p 325-329
    Format: text
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  • 10
    Publication Date: 2013-08-31
    Description: Currently, the light source most commonly used in animal habitat lighting is cool white fluorescent (CWF) light. It was the objective of this study to evaluate a novel LED light source for use in animal habitat lighting by comparing its effectiveness to CWF light in producing and maintaining a normal circadian entrainment. The LED and CWF lights had similar spectral power distributions. Sprague-Dawley rats (175-350 g) were kept individually in metabolic cages, under a strict lighting control: 4 days of acclimation at 12:12 LD, 14 days of 12:12 LD, 14 days of 24:0 LD (free-run), and finally 12:12 LD. Food and water were provided ad libitum. Three behavioral parameters were monitored continuously: gross locomotor activity, drinking, and feeding. Combined mean free run periods (tau) were (mean +/- SEM): 24.6 +/- 0.1 and 24.7 +/- 0.2 at 0.1 lux, 25.5 +/- 0.1 and 25.7 +/- 0.1 at 1.0 lux, 25.3 +/- 0.2 and 25.4 +/- 0.2 at 10 lux, 25.8 +/- 0.1 and 25.9 +/- 0.1 at 40 lux, and 25.9 +/- 0.1 and 25.9 +/- 0.1 at 80 lux, CWF and LED respectively. ANOVA found a significant effect (p 〈 0.05) due to light level, but no difference in tau between rats exposed to constant CWF light and rats exposed to constant LED light. This study has shown that LED light can produce the same entrainment pattern as a conventional CWT light at similar intensities (0.1, 1, 10, 40, and 80 lux). LED light sources may be a suitable replacement for conventional light sources used in animal habitat lighting while providing many mechanical and economical advantages.
    Keywords: Life Sciences (General)
    Format: application/pdf
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